Quantum-state–selective electron recombination studies suggest enhanced abundance of primordial HeH +

Author:

Novotný Oldřich1ORCID,Wilhelm Patrick1ORCID,Paul Daniel1ORCID,Kálosi Ábel12ORCID,Saurabh Sunny1,Becker Arno1,Blaum Klaus1ORCID,George Sebastian13ORCID,Göck Jürgen1,Grieser Manfred1,Grussie Florian1,von Hahn Robert1,Krantz Claude1,Kreckel Holger1ORCID,Meyer Christian1ORCID,Mishra Preeti M.1,Muell Damian1ORCID,Nuesslein Felix1,Orlov Dmitry A.1,Rimmler Marius1ORCID,Schmidt Viviane C.1ORCID,Shornikov Andrey1,Terekhov Aleksandr S.4,Vogel Stephen1,Zajfman Daniel5ORCID,Wolf Andreas1ORCID

Affiliation:

1. Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.

2. Faculty of Mathematics and Physics, Charles University, 18000 Praha, Czech Republic.

3. Institut für Physik, Universität Greifswald, 17487 Greifswald, Germany.

4. Rzhanov Institute of Semiconductor Physics, Novosibirsk 630090, Russia.

5. Weizmann Institute of Science, Rehovot 76100, Israel.

Abstract

Enhanced abundance of primordial HeH + Though only recently detected in space, the helium hydride ion (HeH + ) is thought to be the first molecule ever to have formed in the early Universe. Novotný et al. report state-specific rate coefficients for the dissociative reaction of HeH + with electrons, obtained using a cryogenic ion storage ring combined with a merged electron beam (see the Perspective by Bovino and Galli). They detect substantial rotational dependence and a decrease of the rates for the lowest states of HeH + , far below the values listed in astrochemistry databases and those previously applied in early-Universe models. These results suggest high abundance of this important primordial molecule at redshifts of first star and galaxy formation. Science , this issue p. 676 ; see also p. 639

Funder

European Research Council

Deutsche Forschungsgemeinschaft

Max-Planck-Gesellschaft

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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